The production of \(^7\) Li during nova eruptions has been predicted
theoretically (e.g. [1]}, [2]}, [3]}) and confirmed observationally (e.g.
[4]}, [5]}, [6]}).
Up to \(\sim \) 1\(\times \) 10\(^{-5}\)  of the whole mass of the ejecta can be in the
form of \(^7\) Li, actually \(^7\) Be that will decay into \(^7\) Li. The large
amounts produced during outbursts (especially those occurring on white
dwarfs of the Carbon-Oxygen type), suggests that novae could be the main
producer of \(^7\) Li in the Milky Way [7]}.
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